The Sloan Digital Sky Survey Quasar Lens Search III Constraints on dark energy from the third data release quasar lens catalog

• The SDSS-III's Baryon Oscillation Spectroscopic Survey (BOSS) will map the spatial distribution of luminous red galaxies (LRGs) and quasars to detect the characteristic

3. Estimate the physical properties of the system: mass density slope of the lens galaxy γ, projected dark matter mass fraction within the Einstein radius M dark /M lens ,

In the previous sections we have shown how astronomical alignments and solar hierophanies – with a common interest in the solstices − were substantiated in the

By comparing the predicted rotation curves with observations of dwarf and low surface brightness galaxies, we show that the pressure from dark matter annihilation may improve

Whether an XDQSOz PQSO (z>0.9) selection alone is suf ficient to meet the eBOSS targeting goal of 58 deg −2 quasars is investigated in Figure 3, where the sky density of

teriza por dos factores, que vienen a determinar la especial responsabilidad que incumbe al Tribunal de Justicia en esta materia: de un lado, la inexistencia, en el

As we have seen, even though the addition of a cosmological constant to Einstein’s eld equations may be the simplest way to obtain acceleration, it has its caveats. For this rea-

Paper I: The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: modelling the clustering and halo occupation distribution of BOSS CMASS galaxies in